The Nucleon Axial-Vector Form Factor at the Physical Point with the - - PowerPoint PPT Presentation

the nucleon axial vector form factor at the physical
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The Nucleon Axial-Vector Form Factor at the Physical Point with the - - PowerPoint PPT Presentation

The Nucleon Axial-Vector Form Factor at the Physical Point with the HISQ Ensembles Aaron Meyer (asmeyer2012@uchicago.edu) University of Chicago/Fermilab May 1-2, 2015 USQCD All-Hands Meeting Fermilab Lattice/MILC Collaborations + Richard


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SLIDE 1

The Nucleon Axial-Vector Form Factor at the Physical Point with the HISQ Ensembles

Aaron Meyer (asmeyer2012@uchicago.edu) University of Chicago/Fermilab May 1-2, 2015 USQCD All-Hands Meeting Fermilab Lattice/MILC Collaborations + Richard Hill (UChicago) + Ruizi Li (Wuppertal) with support from URA Visiting Scholars Program, DOE SCGSR

1 / 19

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SLIDE 2

Calculation Overview

We will use MILC HISQ 2+1+1 ensembles at Mπ = 135 MeV with 3 lattice spacings Our primary objectives are to calculate:

  • gA, FA(q2) → Neutrino CCQE/Oscillation Studies
  • gV , FV (q2) → Validation Check/Proton Radius Puzzle

As a byproduct, we will also get:

  • FP(q2) → ντ interaction cross section
  • gS → Dark matter searches and µ to e conversion
  • gT → New physics in neutron β decay

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SLIDE 3

Motivation

Neutrino physics needs a better understanding of axial form factor:

  • Model-dependent shape parameterization introduces

systematic uncertainties and underestimates errors

  • Nuclear effects entangled with nucleon cross sections
  • Measurement of oscillation parameters depends on nuclear

models and nucleon form factors

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SLIDE 4

Circle of Uncertainty

Nucleon-level/Nucleus-level effects entangled Measurements of observables are model-dependent LQCD acts as disruptive techology to break the cycle

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SLIDE 5

Discrepancies in the Axial-Vector Form Factor

Most analyses assume the “Dipole form factor”: F dipole

A

(q2) = gA 1

  • 1 − q2

m2

A

2 (1) Dipole is an ansatz: unmotivated in interesting energy range → uncontrolled systematics and underestimated uncertainties Essential to replace ansatz with model-independent ab-initio calculation from Lattice QCD MiniBooNE Collab., PHYS REV D 81, 092005 (2010)

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SLIDE 6

Calculation Method

⊥(q2) = Aµ(q2) − qµ

q2 q · A (2) FA

  • q2

up(q)γµ

⊥γ5un(0) =

N′| ZAAa

⊥ µ

  • q2

|N 0| ZAAa

0 (0) |πa ω2

  • this work

0| 2 ˆ mPa (0) |πa Mπ

  • (ref)

ω2

  • a→0

(3) Calculation applies for q2 = 0 without issue Renormalization cancels Will fit form factor using a model-independent parameterization: z(t; t0, tc) = √tc − t − √tc − t0 √tc − t + √tc − t0 FA(z) =

  • n=0

anzn (4) As validated by B meson physics, only a few coefficients necessary to accurately represent data

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SLIDE 7

Current Calculations of gA

Other collaborations have at most one ensemble for one lattice spacing at physical pion mass (See backup slides for references)

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SLIDE 8

Advantages of HISQ

  • No explicit chiral symmetry breaking in m→0 limit
  • No exceptional configurations
  • No chiral extrapolation (physical π mass only)
  • Several lattice spacings (true continuum extrapolation)
  • Can go to high statistics easily (HISQ is fast)

1 1 5 2 2 5 3 3 5

Mπ [MeV]

0.05 0.1 0.15 0.2

a (fm)

completed in progress planned Mπ=135 MeV 8 / 19

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SLIDE 9

Taste Mixing

SU(2)I × GTS irrep #N #∆ 3

2, 8

  • 3

2 3

2, 8′

2 3

2, 16

  • 1

3 1

2, 8

  • 5

1 1

2, 8′

1 1

2, 16

  • 3

4 (J. A. Bailey) Group theory for staggered baryons is under control 3-point functions use same operator basis as 2-point functions Set of 4 operators to generate a 4 × 4 matrix of correlators for variational analysis Irrep 3

2, 16

  • chosen because of number of N/∆ states

Can get priors from fitting different taste ∆ states from 3

2, 8′

and 1

2, 8′

  • perators

9 / 19

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SLIDE 10

Finite Size Effects

(See last slide for references)

Doing as well as other calculations at physical masses MILC g − 2 proposal to generate a = 0.15 fm ensemble at larger L → can use for finite volume study Estimate finite-size effects with χPT and L¨ uscher methodology

10 / 19

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SLIDE 11

Excited State Removal

Will employ a number of techniques to remove excited states:

  • N-state excited state analysis using Gaussian priors
  • Variational method, cf. arXiv:1411.4676 [hep-lat] and
  • R. Li (IU Ph.D. Thesis)
  • Random wall sources
  • Gaussian smearing at source and sink
  • Multiple source/sink separations
  • Simultaneous fitting of 2-point/3-point functions
  • Signal to noise optimization
  • Data will be analyzed with a blinding factor applied to the

3-point function MILC Collaboration, R. Li offer expertise for many of these methods

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SLIDE 12

Effective Mass Plots

a ≈ 0.12 fm, mℓ

ms ≈ 0.16

a ≈ 0.09 fm, mℓ

ms ≈ 0.22

(R. Li, Ph.D. Thesis) Variational method has been tested/verified on HISQ Plateau after 3-4/4-5 timeslices → 3-point source/sink separation approximately 2× larger → Scaled with physical dimensions Excited states are under control

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SLIDE 13

Resource Request

≈ a N3

S × NT

Nconfs 8Nζ(Np + Nsink) fm M Jpsi-core-hr 0.15 323 × 48 1000 0.57 0.12 483 × 64 1000 4.71 0.09 643 × 96 1047 23.07 total 28.35 8 staggered baryon cube corners Nζ color vectors (using 3) Np momenta (using 3) Nsink sinks (source/sink separations) (using 2) = 120 inversions total per gauge configuration

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SLIDE 14

Conclusions

Neutrino physics is subject to underestimated and model-dependent systematics → To reduce systematics from modeling, need to understand nuclear physics → To understand nuclear physics, need to understand nucleon-level cross sections HISQ ensembles will produce a high-statistics calculation of the axial form factor at physical pion mass and provide a model-independent description of nucleon-level physics Other areas of study to address in the future to further the Fermilab neutrino program:

  • νℓN → νℓN′
  • N-∆ transition currents
  • νℓN → πℓN′
  • νℓN → πℓΣ

14 / 19

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SLIDE 15

Backup Slides

15 / 19

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SLIDE 16

Nuclear Effects

Nuclear effects not well understood → Models which are best for one measurement are worst for another Need to break FA/nuclear model entanglement A νµ A′ p µ− (assumed mA = 0.99 GeV, reference hyperlinks online) NuWro Model RFG RFG+ assorted (χ2/DOF) [GENIE] TEM

  • thers

leptonic(rate) 3.5 2.4 2.8-3.7 leptonic(shape) 4.1 1.7 2.1-3.8 hadronic(rate) 1.7[1.2] 3.9 1.9-3.7 hadronic(shape) 3.3[1.8] 5.8 3.6-4.8

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SLIDE 17

Form Factor q2 Interpolation

z-Expansion is a model-independent description of the axial form factor t = q2 = −Q2 tc = 9m2

π

z(t; t0, tc) = √tc − t − √tc − t0 √tc − t + √tc − t0 (5) FA(z) =

  • n=0

anzn (6) Maps kinematically allowed region (t ≤ 0) to within z = ±1 From B meson physics, only a few coefficients necessary to accurately represent data z-Expansion implemented in GENIE, to be released soon [autumn]

17 / 19

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SLIDE 18

Error Budgets

LBNE Experiment

18 / 19

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SLIDE 19

gA Calculation references

ETMC

  • S. Dinter et al. arXiv:1108.1076 [hep-lat]

PNDME

  • T. Bhattacharya et al. arXiv:1306.5435 [hep-lat]
  • T. Bhattacharya, R. Gupta, and B. Yoon arXiv:1503.05975 [hep-lat]
  • R. Gupta, T. Bhattacharya, A. Joseph, H.-W. Lin, and B. Yoon arXiv:1501.07639 [hep-lat]

CSSM

  • B. J. Owen et al., arXiv:1212.4668 [hep-lat]

χQCD Y.-B. Yang, M. Gong, K.-F. Liu, and M. Sun arXiv:1504.04052 [hep-ph] LHP(BMW)

  • J. Green et al., arXiv:1211.0253 [hep-lat]
  • S. N. Syritsyn et al., arXiv:0907.4194 [hep-lat]
  • S. D¨

urr et al. arXiv:1011.2711 [hep-lat] LHP(asqtad)

  • S. N. Syritsyn, Exploration of nucleon structure in lattice QCD with chiral quarks, Ph.D. thesis, Massachusetts

Institute of Technology (2010). LHP-RBC

  • S. Syritsyn et al. arXiv:1412.3175 [hep-lat]

RBC-UKQCD

  • S. Ohta arXiv:1309.7942 [hep-lat]

UKQCD-QCDSF

  • M. G¨
  • ckeler et al. arXiv:1102.3407 [hep-lat]

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